STUDY OF MUONS FROM THE DIRECTION OF CYGNUS-X-3 USING AN UNDERGROUND PROPORTIONAL-TUBE ARRAY

被引:3
作者
KOCHOCKI, JA
ALLISON, WWM
ALNER, GJ
AMBATS, I
AYRES, DS
BALKA, LJ
BARR, GD
BARRETT, WL
BENJAMIN, D
BORDER, P
BROOKS, CB
COBB, JH
COCKERILL, DJA
COOVER, K
COURANT, H
DAHLIN, B
DASGUPTA, U
DAWSON, JW
EDWARDS, VW
FIELDS, TH
KIRBYGALLAGHER, LM
GARCIAGARCIA, C
GILES, RH
GOODMAN, MC
HELLER, K
HEPPELMAN, S
HILL, N
HOFTIEZER, JH
JANKOWSKI, DJ
JOHNS, K
JOYCE, T
KAFKA, T
LITCHFIELD, PJ
LOPEZ, FV
LOWE, M
MANN, WA
MARSHAK, ML
MAY, EN
MCMASTER, L
MILBURN, RH
MILLER, W
NAPIER, A
OLIVER, WP
PEARCE, GF
PERKINS, DH
PETERSON, EA
PRICE, LE
ROBACK, D
ROSEN, DB
RUDDICK, K
机构
[1] UNIV OXFORD,OXFORD OX1 3RH,ENGLAND
[2] ARGONNE NATL LAB,ARGONNE,IL 60439
[3] UNIV MINNESOTA,MINNEAPOLIS,MN 55455
[4] RUTHERFORD APPLETON LAB,DIDCOT OX11 0QX,OXON,ENGLAND
来源
PHYSICAL REVIEW D | 1990年 / 42卷 / 09期
关键词
D O I
10.1103/PhysRevD.42.2967
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
From July 1987 through March 1988 an array of proportional wire modules was operated as a muon detector at a depth of 2090 meters water equivalent in the Soudan mine in northern Minnesota. A spatial angular resolution of 1.2°was achieved for muon tracking. A clean sample of 1.02×105 muon trajectories recorded underground is used to search for an excess flux of muons from the direction of Cygnus X-3. For muons within the phase interval [0.6, 0.9] of the source's 4.8-h period, 90%-C.L. upper limits for fluxes arriving within 3°and 1.5°half-angle cones centered on the Cygnus X-3 direction are 8.5×1011 cm-2s-1 and 3.1×10-11 cm-2s-1, respectively. © 1990 The American Physical Society.
引用
收藏
页码:2967 / 2973
页数:7
相关论文
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